The moment of inertia is crucial for understanding the rotational dynamics of objects.
A rotation axis not going through the center of mass requires special consideration to determine the moment of inertia.
The Parallel Axis Theorem is used to calculate the moment of inertia of an object when the axis of rotation is not through its center of mass.
Statement of the Theorem: [ I = I_{cm} + m imes d^2 ]
Where:
( I ) = moment of inertia about any parallel axis
( I_{cm} ) = moment of inertia about the center of mass
( m ) = total mass of the object
( d ) = distance from the center of mass to the new axis
Example with a uniform rod:
If the rod's center of mass is at ( l/2 ), then ( d = l/2 ) for rotation about one end.
Moment of inertia through the center of mass: ( I_{cm} = \frac{1}{12} m l^2 )
Updated calculation yields ( I = \frac{1}{3} m l^2 ).
Torque (( \tau )) is the rotational equivalent of force. It is defined as:
( \tau = r \times f )
The direction of torque is determined using the right-hand rule:
Align fingers along the radial vector (r), curl towards the force direction (f), thumb points in the torque direction.
Vector Notation:
The order matters: ( \tau
eq f \times r )
To compute torque from two vectors:
Use a 3x3 determinant format involving unit vectors ( i, j, k ).
Example determinant: [ \begin{vmatrix} i & j & k \ r_x & r_y & r_z \ f_x & f_y & f_z \end{vmatrix} ]
Important to calculate each component of the torque vector correctly and to maintain sign conventions.
Equations of motion for linear and rotational dynamics link through the tensions in string systems:
For a mass sliding on a surface, apply Newton's second law:
( m_1 g - T_1 = m_1 a ) for the mass in free fall.
( T_2 = m_2 a ) for the sliding mass.
The sum of torques relates to angular acceleration:
( \tau = I \alpha )
Relate angular acceleration to linear acceleration using ( a = \alpha r ).
Given:
Mass ( m_1 ) hanging vertically, mass ( m_2 ) on a surface, and a pulley of radius ( r ).
Free body diagram includes forces: gravitational force and tension.
Establish free body equations for each mass:
Combine forces to derive equations for tensions in strings.
Solve for the moment of inertia using:
( I = \frac{r^2 (T_1 - T_2)}{a} ) where ( T_1 ) and ( T_2 ) are tensions derived from their respective linear equations.
Example results yielded an inertia of ( 0.2 , ext{kg m}^2 ).
Understanding the moment of inertia, parallel axis theorem, and torque calculations is fundamental in addressing problems involving rotation and dynamics.